Home > Publications database > Evidence for $\gamma$-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations > print

001     481249
005     20250724151705.0
024 7 _ |a 10.1051/0004-6361/202243096
|2 doi
024 7 _ |a HESS:2022baw
|2 INSPIRETeX
024 7 _ |a inspire:2012097
|2 inspire
024 7 _ |a 0004-6361
|2 ISSN
024 7 _ |a 1432-0746
|2 ISSN
024 7 _ |a arXiv:2201.05839
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2022-04260
|2 datacite_doi
024 7 _ |a altmetric:121171627
|2 altmetric
024 7 _ |a WOS:000851302600006
|2 WOS
024 7 _ |a openalex:W4221148146
|2 openalex
037 _ _ |a PUBDB-2022-04260
041 _ _ |a English
082 _ _ |a 520
088 _ _ |a arXiv:2201.05839
|2 arXiv
100 1 _ |a Aharonian, F.
|0 F.Aharonian.1
|b 0
245 _ _ |a Evidence for $\gamma$-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations
260 _ _ |a Les Ulis
|c 2022
|b EDP Sciences
336 7 _ |a article
|2 DRIVER
336 7 _ |a Output Types/Journal article
|2 DataCite
336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1659960074_920
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
|2 BibTeX
336 7 _ |a JOURNAL_ARTICLE
|2 ORCID
336 7 _ |a Journal Article
|0 0
|2 EndNote
520 _ _ |a Observations with imaging atmospheric Cherenkov telescopes (IACTs) have enhanced our knowledge of nearby supernova (SN) remnants with ages younger than 500 yr by establishing Cassiopeia A and the remnant of Tycho’s SN as very-high-energy (VHE) γ-ray sources. The remnant of Kepler’s SN, which is the product of the most recent naked-eye SN in our Galaxy, is comparable in age to the other two, but is significantly more distant. If the γ-ray luminosities of the remnants of Tycho’s and Kepler’s SNe are similar, then the latter is expected to be one of the faintest γ-ray sources within reach of the current generation IACT arrays. Here we report evidence at a statistical level of 4.6σ for a VHE signal from the remnant of Kepler’s SN based on deep observations by the High Energy Stereoscopic System (H.E.S.S.) with an exposure of 152 h. The measured integral flux above an energy of 226 GeV is ∼0.3% of the flux of the Crab Nebula. The spectral energy distribution (SED) reveals a γ-ray emitting component connecting the VHE emission observed with H.E.S.S. to the emission observed at GeV energies with Fermi-LAT. The overall SED is similar to that of the remnant of Tycho’s SN, possibly indicating the same nonthermal emission processes acting in both these young remnants of thermonuclear SNe.
536 _ _ |a 613 - Matter and Radiation from the Universe (POF4-613)
|0 G:(DE-HGF)POF4-613
|c POF4-613
|f POF IV
|x 0
588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a gamma ray: emission
|2 INSPIRE
650 _ 7 |a energy: high
|2 INSPIRE
650 _ 7 |a Cherenkov counter: atmosphere
|2 INSPIRE
650 _ 7 |a supernova
|2 INSPIRE
650 _ 7 |a energy spectrum
|2 INSPIRE
650 _ 7 |a VHE
|2 INSPIRE
650 _ 7 |a HESS
|2 INSPIRE
650 _ 7 |a GeV
|2 INSPIRE
650 _ 7 |a flux
|2 INSPIRE
650 _ 7 |a spectral
|2 INSPIRE
650 _ 7 |a imaging
|2 INSPIRE
650 _ 7 |a GLAST
|2 INSPIRE
650 _ 7 |a statistical
|2 INSPIRE
650 _ 7 |a galaxy
|2 INSPIRE
650 _ 7 |a gamma rays: general
|2 autogen
650 _ 7 |a supernovae: individual: Kepler
|2 autogen
650 _ 7 |a gamma-rays: general
|2 autogen
650 _ 7 |a supernovae: individual: Kepler’s SN
|2 autogen
650 _ 7 |a ISM: supernova remnants
|2 autogen
650 _ 7 |a radiation mechanisms: non-thermal
|2 autogen
693 _ _ |0 EXP:(DE-H253)HESS-20170101
|5 EXP:(DE-H253)HESS-20170101
|e High Energy Stereoscopic System
|x 0
700 1 _ |a Benkhali, F. Ait
|0 F.A.Benkhali.1
|b 1
700 1 _ |a Anguner, E. O.
|b 2
700 1 _ |a Ashkar, H.
|0 H.Ashkar.1
|b 3
700 1 _ |a Backes, M.
|0 M.Backes.1
|b 4
700 1 _ |a Martins, V. Barbosa
|0 P:(DE-H253)PIP1085491
|b 5
700 1 _ |a Batzofin, R.
|0 R.Batzofin.1
|b 6
700 1 _ |a Becherini, Y.
|0 Y.Becherini.1
|b 7
700 1 _ |a Berge, D.
|0 P:(DE-H253)PIP1080570
|b 8
700 1 _ |a Bernloehr, K.
|0 K.Bernloehr.1
|b 9
700 1 _ |a Boettcher, M.
|b 10
700 1 _ |a Boisson, C.
|b 11
700 1 _ |a Bolmont, J.
|0 P:(DE-H253)PIP1005246
|b 12
700 1 _ |a de Lavergne, M. de Bony
|0 M.d.de.Lavergne.1
|b 13
700 1 _ |a Breuhaus, M.
|0 M.Breuhaus.1
|b 14
700 1 _ |a Brose, R.
|b 15
700 1 _ |a Brun, F.
|b 16
700 1 _ |a Bulik, T.
|0 T.Bulik.1
|b 17
700 1 _ |a Bylund, T.
|0 T.Bylund.4
|b 18
700 1 _ |a Cangemi, F.
|0 F.Cangemi.3
|b 19
700 1 _ |a Caroff, S.
|0 S.Caroff.1
|b 20
700 1 _ |a Casanova, S.
|0 S.Casanova.1
|b 21
700 1 _ |a Cerruti, M.
|0 M.Cerruti.1
|b 22
700 1 _ |a Chand, T.
|0 T.Chand.2
|b 23
700 1 _ |a Chen, A.
|b 24
700 1 _ |a Chibueze, O.
|0 J.O.Chibueze.1
|b 25
700 1 _ |a Cotter, G.
|0 G.Cotter.8
|b 26
700 1 _ |a Cristofari, P.
|0 P.Cristofari.1
|b 27
700 1 _ |a Mbarubucyeye, Jean Damascene
|0 P:(DE-H253)PIP1090733
|b 28
|u desy
700 1 _ |a Devin, J.
|0 J.Devin.3
|b 29
700 1 _ |a Djannati-Atai, A.
|0 A.Djannati.Atai.1
|b 30
700 1 _ |a Dmytriiev, A.
|0 A.Dmytriiev.3
|b 31
700 1 _ |a Egberts, K.
|b 32
700 1 _ |a Einecke, S.
|0 S.Einecke.1
|b 33
700 1 _ |a Ernenwein, J.-P.
|0 J.P.Ernenwein.4
|b 34
700 1 _ |a Feijen, K.
|0 K.Feijen.1
|b 35
700 1 _ |a Fiasson, A.
|0 A.Fiasson.4
|b 36
700 1 _ |a de Clairfontaine, G. Fichet
|0 G.F.de.Clairfontaine.1
|b 37
700 1 _ |a Fontaine, G.
|0 G.Fontaine.1
|b 38
700 1 _ |a Funk, S.
|b 39
700 1 _ |a Gabici, S.
|0 S.Gabici.1
|b 40
700 1 _ |a Gallant, Y. A.
|b 41
700 1 _ |a Ghafourizadeh, S.
|0 S.Ghafourizadeh.2
|b 42
700 1 _ |a Giavitto, Gianluca
|0 P:(DE-H253)PIP1018949
|b 43
|u desy
700 1 _ |a Giunti, L.
|0 L.Giunti.1
|b 44
700 1 _ |a Glawion, D.
|0 D.Glawion.3
|b 45
700 1 _ |a Glicenstein, J. F.
|0 J.F.Glicenstein.1
|b 46
700 1 _ |a Grondin, M.-H.
|0 M.H.Grondin.2
|b 47
700 1 _ |a Hoerbe, M.
|0 M.R.Hoerbe.1
|b 48
700 1 _ |a Hofmann, W.
|b 49
700 1 _ |a Holch, Tim Lukas
|0 P:(DE-H253)PIP1022858
|b 50
|u desy
700 1 _ |a Holler, M.
|b 51
700 1 _ |a Horns, D.
|0 P:(DE-H253)PIP1006257
|b 52
700 1 _ |a Huang, Zhiqiu
|0 Zheng.Huang.1
|b 53
700 1 _ |a Jamrozy, M.
|0 M.Jamrozy.9
|b 54
700 1 _ |a Joshi, V.
|b 55
700 1 _ |a Jung-Richardt, I.
|0 I.JungRichardt.2
|b 56
700 1 _ |a Kasai, E.
|b 57
700 1 _ |a Katarzynski, K.
|0 K.Katarzynski.4
|b 58
700 1 _ |a Katz, U.
|0 U.F.Katz.1
|b 59
700 1 _ |a Khelifi, B.
|0 B.Khelifi.1
|b 60
700 1 _ |a Kluzniak, W.
|0 W.Kluzniak.2
|b 61
700 1 _ |a Komin, Nu.
|0 N.Komin.1
|b 62
700 1 _ |a Kosack, K.
|b 63
700 1 _ |a Kostunin, D.
|0 P:(DE-H253)PIP1085187
|b 64
700 1 _ |a Lemiere, A.
|0 A.Lemiere.1
|b 65
700 1 _ |a Lemoine-Goumard, M.
|0 M.Lemoine.Goumard.1
|b 66
700 1 _ |a Lenain, J.-P.
|0 J.P.Lenain.1
|b 67
700 1 _ |a Leuschner, F.
|0 F.Leuschner.1
|b 68
700 1 _ |a Lohse, T.
|b 69
700 1 _ |a Luashvili, A.
|0 A.Luashvili.1
|b 70
700 1 _ |a Lypova, I.
|b 71
700 1 _ |a Mackey, J.
|0 J.Mackey.2
|b 72
700 1 _ |a Malyshev, D.
|0 D.Malyshev.3
|b 73
700 1 _ |a Marandon, V.
|0 V.Marandon.1
|b 74
700 1 _ |a Marchegiani, P.
|0 P.Marchegiani.2
|b 75
700 1 _ |a Marcowith, A.
|0 A.Marcowith.1
|b 76
700 1 _ |a Marti-Devesa, G.
|0 G.MartiDevesa.1
|b 77
700 1 _ |a Marx, R.
|b 78
700 1 _ |a Maurin, G.
|0 Gilles.Maurin.1
|b 79
700 1 _ |a Meintjes, P. J.
|0 P.J.Meintjes.5
|b 80
700 1 _ |a Meyer, M.
|b 81
700 1 _ |a Mitchell, A.
|b 82
700 1 _ |a Moderski, R.
|0 R.Moderski.14
|b 83
700 1 _ |a Mohrmann, L.
|0 P:(DE-H253)PIP1012638
|b 84
700 1 _ |a Montanari, A.
|b 85
700 1 _ |a Moulin, E.
|b 86
700 1 _ |a Muller, J.
|b 87
700 1 _ |a Nakashima, K.
|0 K.Nakashima.1
|b 88
700 1 _ |a de Naurois, M.
|0 M.de.Naurois.1
|b 89
700 1 _ |a Nayerhoda, A.
|0 A.Nayerhoda.3
|b 90
700 1 _ |a Niemiec, J.
|b 91
700 1 _ |a Noel, A. Priyana
|b 92
700 1 _ |a O'Brien, P.
|0 P.OBrien.7
|b 93
700 1 _ |a Ohm, Stefan
|0 P:(DE-H253)PIP1021898
|b 94
|u desy
700 1 _ |a Olivera-Nieto, L.
|0 L.OliveraNieto.1
|b 95
700 1 _ |a Wilhelmi, E. de Ona
|0 E.de.Ona.Wilhelmi.1
|b 96
700 1 _ |a Ostrowski, M.
|b 97
700 1 _ |a Panny, S.
|0 S.Panny.1
|b 98
700 1 _ |a Panter, M.
|0 M.Panter.3
|b 99
700 1 _ |a Parsons, R. D.
|b 100
700 1 _ |a Peron, G.
|0 G.Peron.2
|b 101
700 1 _ |a Poireau, V.
|0 V.Poireau.1
|b 102
700 1 _ |a Prokhorov, D. A.
|0 D.A.Prokhorov.1
|b 103
|e Corresponding author
700 1 _ |a Puehlhofer, G.
|0 G.PUEHLHOFER.1
|b 104
700 1 _ |a Punch, M.
|0 M.Punch.1
|b 105
700 1 _ |a Quirrenbach, A.
|0 A.Quirrenbach.8
|b 106
700 1 _ |a Reichherzer, P.
|0 P.Reichherzer.2
|b 107
700 1 _ |a Reimer, A.
|b 108
700 1 _ |a Reimer, O.
|b 109
700 1 _ |a Renaud, M.
|0 M.Renaud.7
|b 110
700 1 _ |a Reville, B.
|0 B.Reville.1
|b 111
700 1 _ |a Rieger, F.
|b 112
700 1 _ |a Rowell, G.
|0 Gavin.P.Rowell.1
|b 113
700 1 _ |a Rudak, B.
|0 B.Rudak.11
|b 114
700 1 _ |a Ricarte, H. Rueda
|0 H.R.Ricarte.1
|b 115
700 1 _ |a Sahakian, V.
|0 Vardan.Sahakian.1
|b 116
700 1 _ |a Sailer, S.
|0 S.Sailer.1
|b 117
700 1 _ |a Salzmann, H.
|b 118
700 1 _ |a Sanchez, D. A.
|b 119
700 1 _ |a Santangelo, A.
|0 A.Santangelo.21
|b 120
700 1 _ |a Sasaki, M.
|0 M.Sasaki.2
|b 121
700 1 _ |a Schafer, J.
|b 122
700 1 _ |a Schussler, F.
|0 F.Schuessler.1
|b 123
700 1 _ |a Schutte, H. M.
|0 H.M.Schutte.1
|b 124
700 1 _ |a Schwanke, U.
|b 125
700 1 _ |a Shapopi, J. N. S.
|0 J.N.S.Shapopi.1
|b 126
700 1 _ |a Simoni, R.
|0 R.Simoni.2
|b 127
700 1 _ |a Sol, H.
|0 H.Sol.7
|b 128
700 1 _ |a Specovius, A.
|0 A.Specovius.1
|b 129
700 1 _ |a Spencer, S.
|b 130
700 1 _ |a Stawarz, L.
|0 L.Stawarz.1
|b 131
700 1 _ |a Steinmassl, S.
|0 S.Steinmassl.1
|b 132
700 1 _ |a Steppa, C.
|b 133
700 1 _ |a Sushch, I.
|b 134
700 1 _ |a Takahashi, T.
|b 135
700 1 _ |a Tanaka, T.
|b 136
700 1 _ |a Taylor, A. M.
|0 P:(DE-H253)PIP1080492
|b 137
700 1 _ |a Terrier, R.
|0 R.Terrier.6
|b 138
700 1 _ |a Tsirou, M.
|0 M.Tsirou.2
|b 139
700 1 _ |a Uchiyama, Y.
|0 Y.Uchiyama.3
|b 140
700 1 _ |a Unbehaun, T.
|0 T.Unbehaun.1
|b 141
700 1 _ |a van Eldik, C.
|b 142
700 1 _ |a Veh, J.
|0 J.Veh.2
|b 143
700 1 _ |a Vink, J.
|0 Jacco.Vink.1
|b 144
700 1 _ |a Voelk, H. J.
|0 H.J.Voelk.1
|b 145
700 1 _ |a Wagner, S. J.
|b 146
700 1 _ |a Werner, F.
|0 F.Werner.1
|b 147
700 1 _ |a White, R.
|b 148
700 1 _ |a Wierzcholska, A.
|0 A.Wierzcholska.3
|b 149
700 1 _ |a Wong, Yu Wun
|0 Y.W.Wong.1
|b 150
700 1 _ |a Yusafzai, A.
|0 A.Yusafzai.1
|b 151
700 1 _ |a Zacharias, M.
|b 152
700 1 _ |a Zargaryan, D.
|0 D.Zargaryan.1
|b 153
700 1 _ |a Zdziarski, A. A.
|0 A.A.Zdziarski.1
|b 154
700 1 _ |a Zech, A.
|b 155
700 1 _ |a Zhu, Sylvia Jiechen
|0 P:(DE-H253)PIP1089041
|b 156
|u desy
700 1 _ |a Zouari, S.
|0 S.Zouari.1
|b 157
700 1 _ |a Zywucka, N.
|0 N.Zywucka.3
|b 158
700 1 _ |a H. E. S. S. Collaboration
|0 P:(DE-HGF)0
|b 159
|e Collaboration Author
773 _ _ |a 10.1051/0004-6361/202243096
|g Vol. 662, p. A65 -
|0 PERI:(DE-600)1458466-9
|p A65
|t Astronomy and astrophysics
|v 662
|y 2022
|x 0004-6361
787 0 _ |a Aharonian, F. et.al.
|d 2022
|i IsParent
|0 PUBDB-2022-04266
|r arXiv:2201.05839
|t Evidence for $\gamma$-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations
856 4 _ |y OpenAccess
|u https://bib-pubdb1.desy.de/record/481249/files/AA662%282022%29A65.pdf
856 4 _ |y OpenAccess
|x pdfa
|u https://bib-pubdb1.desy.de/record/481249/files/AA662%282022%29A65.pdf?subformat=pdfa
909 C O |o oai:bib-pubdb1.desy.de:481249
|p openaire
|p open_access
|p VDB
|p driver
|p dnbdelivery
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 5
|6 P:(DE-H253)PIP1085491
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 8
|6 P:(DE-H253)PIP1080570
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 12
|6 P:(DE-H253)PIP1005246
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 28
|6 P:(DE-H253)PIP1090733
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 43
|6 P:(DE-H253)PIP1018949
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 50
|6 P:(DE-H253)PIP1022858
910 1 _ |a External Institute
|0 I:(DE-HGF)0
|k Extern
|b 52
|6 P:(DE-H253)PIP1006257
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 64
|6 P:(DE-H253)PIP1085187
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 94
|6 P:(DE-H253)PIP1021898
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 96
|6 E.de.Ona.Wilhelmi.1
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 137
|6 P:(DE-H253)PIP1080492
910 1 _ |a Deutsches Elektronen-Synchrotron
|0 I:(DE-588b)2008985-5
|k DESY
|b 156
|6 P:(DE-H253)PIP1089041
913 1 _ |a DE-HGF
|b Forschungsbereich Materie
|l Matter and the Universe
|1 G:(DE-HGF)POF4-610
|0 G:(DE-HGF)POF4-613
|3 G:(DE-HGF)POF4
|2 G:(DE-HGF)POF4-600
|4 G:(DE-HGF)POF
|v Matter and Radiation from the Universe
|x 0
914 1 _ |y 2022
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0200
|2 StatID
|b SCOPUS
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0300
|2 StatID
|b Medline
|d 2021-02-02
915 _ _ |a Creative Commons Attribution CC BY 4.0
|0 LIC:(DE-HGF)CCBY4
|2 HGFVOC
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0600
|2 StatID
|b Ebsco Academic Search
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)1150
|2 StatID
|b Current Contents - Physical, Chemical and Earth Sciences
|d 2021-02-02
915 _ _ |a IF >= 5
|0 StatID:(DE-HGF)9905
|2 StatID
|b ASTRON ASTROPHYS : 2019
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0150
|2 StatID
|b Web of Science Core Collection
|d 2021-02-02
915 _ _ |a WoS
|0 StatID:(DE-HGF)0113
|2 StatID
|b Science Citation Index Expanded
|d 2021-02-02
915 _ _ |a OpenAccess
|0 StatID:(DE-HGF)0510
|2 StatID
915 _ _ |a Peer Review
|0 StatID:(DE-HGF)0030
|2 StatID
|b ASC
|d 2021-02-02
915 _ _ |a JCR
|0 StatID:(DE-HGF)0100
|2 StatID
|b ASTRON ASTROPHYS : 2019
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0160
|2 StatID
|b Essential Science Indicators
|d 2021-02-02
915 _ _ |a DBCoverage
|0 StatID:(DE-HGF)0199
|2 StatID
|b Clarivate Analytics Master Journal List
|d 2021-02-02
920 1 _ |0 I:(DE-H253)ZEU-HESS-20140213
|k ZEU-HESS
|l High Energy Steroscopic System
|x 0
980 _ _ |a journal
980 _ _ |a VDB
980 _ _ |a UNRESTRICTED
980 _ _ |a I:(DE-H253)ZEU-HESS-20140213
980 1 _ |a FullTexts

LibraryCollectionCLSMajorCLSMinorLanguageAuthor
Marc 21